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Proceedings Paper

FAME: freeform active mirror experiment
Author(s): Gabby Aitink-Kroes; Tibor Agócs; Chris Miller; Martin Black; Szigfrid Farkas; Sabri Lemared; Felix Bettonvil; David Montgomery; Michel Marcos; Attila Jaskó; Farian van Duffelen; Zalpha Challita; Sandy Fok; Fatemeh Kiaeerad; Emmanuel Hugot; Hermine Schnetler; Lars Venema
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Paper Abstract

FAME is a four-year project and part of the OPTICON/FP7 program that is aimed at providing a breakthrough component for future compact, wide field, high resolution imagers or spectrographs, based on both Freeform technology, and the flexibility and versatility of active systems.

Due to the opening of a new parameter space in optical design, Freeform Optics are a revolution in imaging systems for a broad range of applications from high tech cameras to astronomy, via earth observation systems, drones and defense. Freeform mirrors are defined by a non-rotational symmetry of the surface shape, and the fact that the surface shape cannot be simply described by conicoids extensions, or off-axis conicoids. An extreme freeform surface is a significantly challenging optical surface, especially for UV/VIS/NIR diffraction limited instruments.

The aim of the FAME effort is to use an extreme freeform mirror with standard optics in order to propose an integrated system solution for use in future instruments. The work done so far concentrated on identification of compact, fast, widefield optical designs working in the visible, with diffraction limited performance; optimization of the number of required actuators and their layout; the design of an active array to manipulate the face sheet, as well as the actuator design.

In this paper we present the status of the demonstrator development, with focus on the different building blocks: an extreme freeform thin face sheet, the active array, a highly controllable thermal actuator array, and the metrology and control system.

Paper Details

Date Published: 22 July 2016
PDF: 14 pages
Proc. SPIE 9912, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II, 99121I (22 July 2016); doi: 10.1117/12.2232939
Show Author Affiliations
Gabby Aitink-Kroes, ASTRON (Netherlands)
Tibor Agócs, ASTRON (Netherlands)
Chris Miller, UK Astronomy Technology Ctr. (United Kingdom)
Martin Black, UK Astronomy Technology Ctr. (United Kingdom)
Szigfrid Farkas, Konkoly Observatory (Hungary)
Sabri Lemared, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France)
Felix Bettonvil, ASTRON (Netherlands)
David Montgomery, UK Astronomy Technology Ctr. (United Kingdom)
Michel Marcos, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France)
Attila Jaskó, Konkoly Observatory (Hungary)
Farian van Duffelen, ASTRON (Netherlands)
Zalpha Challita, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France)
Sandy Fok, UK Astronomy Technology Ctr. (United Kingdom)
Fatemeh Kiaeerad, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France)
Emmanuel Hugot, Aix Marseille Univ., CNRS, Lab. d'Astrophysique de Marseille (France)
Hermine Schnetler, UK Astronomy Technology Ctr. (United Kingdom)
Lars Venema, ASTRON (Netherlands)


Published in SPIE Proceedings Vol. 9912:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II
Ramón Navarro; James H. Burge, Editor(s)

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